Observation and analysis of solar spectral radiation in solar eclipse at Mohe

Jianhui Bai; Qinxin Kong

doi:10.1117/12.317737

18 August 1998 Observation and analysis of solar spectral radiation in solar eclipse at Mohe

Jianhui Bai, Qinxin Kong

Proceedings Volume 3501, Optical Remote Sensing of the Atmosphere and Clouds; (1998) https://doi.org/10.1117/12.317737
Event: Asia-Pacific Symposium on Remote Sensing of the Atmosphere, Environment, and Space, 1998, Beijing, China

Abstract

The observation data of solar UV, visible, IR and total radiation during the 9 March 1997 solar eclipse at Mohe have been analyzed, results are the following: during period of solar eclipse, variation trends of solar UV, visible, IR and total radiation were similar, their energy deficits and percentages of energy deficit increased area of the sun 's surface covered by the moon's umbra, and reached the maximum of the solar eclipse. The energy losses of solar UV, visible, IR and total radiation in solar eclipse were 0.09, 0.55, 0.72 and 1.28 MJ/m², respectively. There were still good relationships among solar UV, visible, IR and total radiation during the solar eclipse.

Citation Download Citation

Jianhui Bai and Qinxin Kong "Observation and analysis of solar spectral radiation in solar eclipse at Mohe", Proc. SPIE 3501, Optical Remote Sensing of the Atmosphere and Clouds, (18 August 1998); https://doi.org/10.1117/12.317737

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